This galaxy presents as an elliptical morphology, exhibiting a generally smooth light distribution with a high degree of central concentration. The galaxy's shape is elongated, with a cigar-like appearance. The core displays a reddish hue, possibly indicating an older stellar population and lower levels of star formation activity. The outer regions of the galaxy transition to a bluish color, suggesting the presence of younger stars and the potential for ongoing, albeit low, star formation in these areas. No distinct spiral arms or bar structures are apparent. There is no indication of any major disturbances or interactions with neighboring galaxies, and the galaxy seems isolated.
