The galaxy appears to be a relatively smooth, elliptical structure. Its core exhibits a concentrated, yellowish-white luminosity, suggesting a significant population of older stars. Moving outward from the core, the color transitions to a faint, reddish hue, which is consistent with an aging stellar population. The galaxy lacks any apparent spiral arm structure or dust lanes. The overall shape is somewhat elongated, but not dramatically cigar-shaped. There are no signs of major disturbances or merging events, although there may be subtle irregularities in its outer regions. Overall the structure appears to be fairly consistent with an evolved system.
