This galaxy appears to be a relatively luminous, early-type galaxy. Its overall morphology appears to be smooth, with a dominant, centrally concentrated bulge. The shape of the galaxy is elongated, but not dramatically so, displaying an intermediate ellipticity. There is no clear evidence of spiral arms or a well-defined disk.

The color profile suggests an older stellar population, primarily composed of redder stars, particularly in the central region. However, there are faint blueish or greenish tinges within the galaxy, suggesting either minimal ongoing star formation or a population of younger stars.

A possible minor disturbance can be observed, which could suggest a past or ongoing interaction. Further investigation of the galaxy's immediate environment would be needed to confirm this.
