The galaxy presents as an elliptical or lenticular structure. It appears to be relatively smooth and centrally concentrated, with a diffuse, extended halo surrounding a brighter core. The color profile suggests an older stellar population, with a yellow-red hue dominating the central regions, indicative of evolved stars. There appears to be very little evidence of spiral arm structure or prominent dust lanes. The overall morphology suggests that the galaxy is not currently undergoing significant star formation. There are some minor features that could be a very subtle disk, or features resulting from a minor disturbance, but further investigation would be required to determine the origin of these possible features. The galaxy appears isolated, with no obvious signs of ongoing major mergers or tidal interactions with other galaxies.