The galaxy presents an overall smooth morphology, suggesting it is likely an elliptical or lenticular type. The light distribution appears concentrated towards the center, with a gradual decrease in brightness moving outward. The galaxy's shape appears somewhat elongated, exhibiting a cigar-like form rather than being perfectly spherical. There is no discernible spiral structure or evidence of significant star formation regions. The galaxy's color is primarily a pale yellow-white, indicative of an older stellar population dominated by redder, less massive stars. The light is fairly uniform, with no strong color gradients or distinct features. There might be a slight hint of minor disturbance in the galaxy's structure, potentially a tidal tail or a slight asymmetry. There is no clear evidence of active merging events or major disruptions to the galaxy's overall form.