The galaxy presents as an elliptical morphology, appearing largely featureless and smooth. It exhibits a concentrated central bulge, with luminosity gradually decreasing towards the outer edges. The color profile suggests a dominant population of older stars, as indicated by the yellowish hue. There's no apparent dust lane or spiral arm structure visible, suggesting the cessation of significant star formation activity. The galaxy displays a moderate degree of roundness, trending towards a more spherical shape rather than a highly elongated one. There is no visible evidence of recent or ongoing merger activity or significant tidal disturbances. The object appears as an isolated system within the observed field.
