The galaxy appears to be a relatively smooth, elliptical type. Its morphology is primarily spheroidal, with no immediately discernible spiral arms or bar structure. The light distribution suggests a concentrated central bulge, gradually fading outwards. There is a slight elongation, but overall, the galaxy presents a largely rounded appearance. The color profile indicates a population of older stars, trending towards redder hues, with a hint of younger, bluer stars in the outer regions. There is no obvious evidence of ongoing major mergers or strong tidal disturbances, although there is some subtle asymmetry which may indicate a minor past interaction. The galaxy is unresolved in this image, its diameter is approximately 3 kpc.
