The galaxy presents a generally smooth morphology, appearing largely elliptical. The light distribution is centrally concentrated with a gradual decline in surface brightness away from the core. A slight elongation is observed, deviating from a perfectly circular shape, but it is generally round.

There are no prominent spiral arms or a distinct disk structure evident. The galaxy displays a color gradient; the core shows a yellowish to reddish hue, suggestive of an older stellar population, whereas bluer tinges can be seen in the outskirts of the galaxy which indicates possible recent star formation. 

There is no evidence of major tidal disturbances or ongoing mergers. Some faint irregularities or minor disturbances appear along the edges of the galaxy, hinting at possible past interactions. Overall, the galaxy appears to be a relatively isolated system in a stage of quiescence, but with subtle hints of activity.
