The galaxy presents a generally smooth, elliptical appearance, with some evidence of a disk structure. The overall shape is moderately elongated, appearing somewhere between round and cigar-shaped, but closer to round. The color profile suggests a relatively old stellar population, especially towards the center, which exhibits a yellowish hue, potentially indicating older, redder stars. There are subtle hints of bluer regions in the outer parts of the galaxy, suggesting the presence of younger, hotter stars, implying some ongoing star formation. The galaxy appears somewhat disturbed. There is evidence of a minor interaction or disturbance, although it doesn't appear to be undergoing a major merger or violent disruption.
