The galaxy exhibits an overall elliptical morphology with a smooth light distribution, indicating a relatively homogenous stellar population. The galaxy's core appears bright and concentrated, suggesting a high stellar density. The color profile transitions from a yellowish core to a redder, more diffuse halo. This suggests a potentially older stellar population dominates the outer regions. There are no clearly defined spiral arms or prominent dust lanes visible. Some subtle irregularities in the outer regions could be indicative of minor disturbances, possibly past mergers or interactions.
