The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. It exhibits a yellowish hue, suggesting a population dominated by older stars and potentially lower levels of ongoing star formation. There is little evidence of spiral arms or significant dust lanes. The galaxy appears somewhat spheroidal, with an intermediate ellipticity. No significant tidal disturbances or signs of mergers are apparent in the immediate vicinity. Overall, the galaxy appears to be a mature system, possibly residing on the red sequence.
