The galaxy appears as a relatively smooth, elliptical-like object with a concentrated central bulge. The light distribution suggests a well-defined core, gradually fading outwards. There is minimal evidence of spiral arm structure or significant dust lanes. The overall color profile indicates a population of older stars, evidenced by the yellowish-red hue dominating the galaxy's color. No signs of ongoing major mergers or tidal disturbances are apparent. The galaxy appears to be isolated. Its apparent angular size is relatively small, suggesting that it is a somewhat compact galaxy at a considerable distance.
