The galaxy presents as a relatively smooth, elliptical morphology. Its light distribution is concentrated towards the center, with a gradual decrease in intensity towards the outer regions. There is no clear evidence of distinct spiral arms or a well-defined disk. The overall shape appears somewhat rounded, lacking a highly elongated or cigar-like form. There might be a subtle indication of minor disturbances in the structure, but it is not exhibiting signs of a major merger or significant tidal disruption. The color is dominated by redder wavelengths, suggesting an older stellar population. Star formation rate appears present, although not high.
