This galaxy presents as an elliptical-type galaxy with an overall smooth morphology. The galaxy exhibits a concentrated central bulge that is yellowish in color, suggesting an older stellar population dominates this region. Extending outward from the bulge is a fainter, bluer halo. This may be an indicator of ongoing, albeit low-level, star formation activity.

The galaxy's shape appears elongated, deviating from a perfect circular form. There may be a slight asymmetry in its overall structure, potentially indicating some past or ongoing gravitational interaction. There are no clear signs of prominent spiral arms or a well-defined disk structure. However, there is a smaller object that is close enough that a merger event could be happening.
