The galaxy presents as a single, relatively smooth object with a somewhat spheroidal shape. The light is somewhat evenly distributed across the galaxy, with no obvious bright knots or distinct structures that would suggest the presence of spiral arms or a prominent bar. The galaxy displays a color gradient, appearing bluer towards the central regions, which could indicate a higher concentration of younger, hotter stars there. The overall redder hue of the galaxy suggests a significant population of older stars and potentially dust absorption. There is no clear evidence of ongoing major mergers or tidal disturbances.
