This galaxy presents as a somewhat elliptical, concentrated distribution of light. The core region exhibits a pronounced yellowish hue, suggesting an older stellar population. The isophotes appear relatively smooth, with minimal evidence of spiral arm structure or significant dust lanes. There might be a very slight extension of light visible on one side of the galaxy, though the image resolution limits certainty. The galaxy appears largely undisturbed, showing no clear signs of ongoing major merger activity. The overall morphology indicates a high probability of this galaxy being a relatively massive system with a low star formation rate and a large population of older stars.
