The galaxy presents as a luminous, centrally concentrated object with a generally smooth, elliptical morphology. There is little evidence of spiral arm structure or significant dust lanes. The color appears to be relatively uniform across the galaxy, with a subtle yellowish hue. This suggests a population of older stars, possibly indicating a relatively low star formation rate. The galaxy appears largely undisturbed, with no obvious signs of major mergers or significant tidal interactions. There may be a very slight asymmetry in the outer regions, but further data is required to determine this.
