The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a predominantly elliptical morphology, appearing largely featureless without distinct spiral arms or a prominent bar. The light profile appears centrally peaked with a gradual decrease in intensity towards the outer regions. The galaxy has an overall yellowish-white hue, suggesting a dominant population of older stars. A subtle blueish tint is visible on the periphery, indicating the presence of some younger, bluer stars, but these do not dominate the overall color. There is no obvious dust lane or signs of significant ongoing star formation. The galaxy appears unperturbed, with no clear evidence of tidal interactions or recent merger events. Its shape is closer to round than cigar-shaped. Overall, based on the observed morphology and color, this galaxy is likely an elliptical galaxy, likely composed of an old stellar population with little or no active star formation.
