The galaxy presents as a relatively small, elliptical morphology. It has a smooth and featureless appearance, with no discernible spiral arms or bar structure. The light distribution is concentrated toward the center, with a gradual decrease in brightness towards the outer edges. The galaxy appears moderately flattened, exhibiting an axial ratio of approximately 0.6, indicating a degree of ellipticity. The color is generally redder, suggesting a population of older stars and a lower rate of ongoing star formation. There is no evidence of significant dust lanes or active star-forming regions within the visible structure. The galaxy shows no signs of major tidal disturbances or interactions with other galaxies.
