This galaxy presents an overall irregular morphology, with no discernible spiral arms or elliptical structure immediately apparent. The light distribution appears relatively diffuse and patchy. There is some evidence of what may be a tidal tail or minor disturbance emanating from the galaxy, indicating a potential interaction with another galaxy or recent merger event. The central region shows a slight concentration of light, but no distinct bulge is visible. The color profile suggests a mix of stellar populations; bluer regions indicate ongoing or recent star formation, while redder areas could represent older stellar populations or dust obscuration. There is some evidence of multiple point-like sources within the galaxy, which could be star clusters or individual bright stars. Overall, the galaxy appears to be a relatively low-mass system undergoing some level of dynamical activity. Further investigation is warranted to determine the nature and extent of any interactions and to characterize the star formation history and stellar population content of this galaxy.
