The galaxy exhibits a generally elliptical morphology, appearing largely smooth and rounded, with no discernible spiral arm structure. The light distribution is centrally concentrated, showing a bright, compact core that gradually fades into the outer regions. The galaxy displays a yellow-orange hue in its central regions, suggesting an older stellar population. There is a very faint hint of a disk. The overall impression is of a well-formed galaxy with relatively little ongoing star formation, but a moderate amount as well. There does not appear to be evidence of any major disturbances or ongoing merging activity in this image. The galaxy appears isolated and undisturbed. The size is relatively small.
