The galaxy presents a smooth, elliptical morphology. The central bulge exhibits a bright, concentrated luminosity, indicative of a high stellar density. The overall color appears slightly redder, potentially suggesting an older stellar population and lower ongoing star formation activity. There may be evidence of faint, diffuse outer regions surrounding the central body, but no distinct spiral arms or prominent dust lanes are visible. The shape is generally rounded, with a slight elongation. There is no obvious indication of major interaction or merging activity, although a minor disturbance cannot be entirely ruled out given the image resolution.
