The galaxy presents an elliptical morphology with a smooth light distribution. The central region exhibits a high concentration of luminosity, fading gradually towards the outer edges, showing no distinct spiral arms or features. The galaxy's color is primarily yellow, indicating a likely older stellar population, with limited evidence of ongoing, active star formation. The galaxy appears fairly isolated, with no obvious signs of a major merger event occurring. The absence of significant dust lanes or prominent blue regions further supports the notion of a passively evolving system dominated by older stars.
