The galaxy appears to be a relatively smooth, elliptical-like structure. There is a concentrated central bulge that transitions outward into a less defined halo. The light distribution is fairly even, suggesting a lack of significant spiral arms or distinct features. The galaxy exhibits a yellow to slightly reddish hue, indicating a population of older stars. There is no readily apparent dust or gas obscuring the galaxy's central region, and no signs of active star formation are immediately visible. Overall, the galaxy presents itself as a well-evolved system likely dominated by an older stellar population.
