The galaxy appears to be an elliptical type, exhibiting a generally smooth morphology with minimal discernible features. The light profile shows a concentrated central bulge that diffuses outwards, indicative of a relatively old stellar population. There may be a slightly more defined structure on one side, perhaps a faint spiral arm or tidal tail, but it is only a slight variation from the overall smooth profile. The color is predominately yellow-red, suggesting a population dominated by older, cooler stars. There are some traces of blue light, likely indicative of a limited amount of ongoing star formation, although the estimated star formation rate is very low. The galaxy is moderately large for this distance, with an estimated mass of over ten billion solar masses. There are no clear signs of a major merger event, although the galaxy shows a minor disturbance or interaction. It's shape is between round and in between, but it isn't elongated. 
