The galaxy presents as a moderately bright, elliptical morphology. Its overall color appears to be a pale yellow, indicative of an older stellar population. The central region displays a high degree of luminosity, suggesting a concentrated galactic nucleus. A faint, somewhat indistinct disk feature can be inferred, given its slightly elongated shape. There are indications of a potential minor tidal interaction or disturbance, evidenced by faint, diffuse extensions. Star formation is likely present, but at a relatively low rate, based on the redder hue of the galaxy. Overall, this object appears to be a galaxy undergoing minor mergers and is largely dominated by a smooth profile.
