The galaxy presents a primarily smooth morphology. Its shape appears elliptical, with a slight elongation. A bright central bulge dominates the galaxy's overall luminosity profile, with a noticeable radial decrease in surface brightness moving outward from the core. The color is generally consistent across the galaxy, trending towards a redder hue, suggesting an older stellar population and a relatively low rate of ongoing star formation within the galaxy. The absence of clearly defined spiral arms, dust lanes, or irregular features supports the smooth and elliptical classification. The galaxy does not appear to be significantly disturbed or actively merging.
