The galaxy appears as a centrally concentrated object with a smooth, relatively featureless morphology. It exhibits an elliptical shape, with an axis ratio close to unity, suggesting it is nearly circular when viewed from our line of sight. The color profile indicates a dominant population of older stars, as evidenced by the yellowish-red hue. There is no apparent spiral arm structure or dust lane obscuration visible. The galaxy appears isolated, with no immediate signs of major tidal disturbances or ongoing mergers. A very faint, diffuse halo may be present surrounding the central region, gradually fading into the background sky. Any star formation appears to be minimal.
