The galaxy presents an elliptical morphology with a notable absence of distinct spiral arms. The light distribution appears relatively smooth, with a somewhat brighter, more concentrated central region suggesting a substantial bulge. There is a suggestion of tidal features around the main body of the galaxy, which could indicate either recent or ongoing interactions with a companion. The galaxy exhibits a dominant yellowish-orange hue in its core, likely associated with an older stellar population. Fainter bluish regions are also visible in the outer areas of the galaxy, suggestive of younger stars. The isophotes appear moderately round, and there is an overall impression of a relatively quiescent system. There is the possibility that the galaxy is interacting or merging with one or two smaller objects.