The galaxy presents an elliptical morphology, appearing somewhat elongated but predominantly smooth in texture. There is a slight concentration of light towards the central region, indicating a possible galactic nucleus or a bulge. The color distribution shows a subtle variation, with bluer hues concentrated on the edges of the galaxy, suggesting the presence of younger stellar populations in these regions. Conversely, the core exhibits a more yellow/red hue, which may correspond to an older stellar population. There is no apparent evidence of distinct spiral arms or significant dust lanes. There is a slight disturbance that is visible in the center which might be caused by a small merger. The galaxy is not perfectly symmetrical which may be from the disturbance. The galaxy's overall structure suggests a relatively evolved system with a low star formation rate.
