The galaxy presents as a generally smooth, centrally concentrated object with a slightly elliptical morphology. The color profile suggests a dominant population of older stars, exhibiting a yellowish-red hue. There is no obvious spiral structure or distinct features indicative of ongoing, vigorous star formation, although there are possibly hints of some star formation on the edges. The lack of strong blue emission reinforces the notion of a relatively quiescent galaxy with a low specific star formation rate. There are no visible signs of any interaction with other objects, such as tidal tails or other major disturbances in the surrounding structure.
