The galaxy presents a generally smooth, elliptical morphology. It appears to be primarily composed of an older stellar population, indicated by its reddish-yellow hue. There is no clear evidence of spiral arms or significant dust lanes. The galaxy shows a central bright region likely indicating a dense stellar core or a possible active galactic nucleus. The isophotes exhibit a moderate ellipticity, leaning towards a more rounded shape, with only slight elongation. Overall, the structure suggests an evolved galaxy with a relatively quiescent star formation rate. There is the suggestion of a minor disturbance or tidal tail on one side of the galaxy, which may indicate a past or ongoing interaction with another, smaller galaxy, but it can also be an artifact.
