This galaxy appears to be a relatively smooth, elliptical-like structure, exhibiting a concentrated central bulge that gradually diffuses outward. The light profile suggests a mostly uniform distribution with a slight elongation, more round than cigar shaped. Its color is distinctly reddish-yellow, indicating a likely older stellar population with minimal ongoing star formation. There seems to be some evidence of a possible interaction or minor disturbance visible in the slight irregularities of the outer halo, although a clear merging event is not immediately obvious in the image. The galaxy shows an estimated effective radius indicating a substantial physical size.
