The galaxy presents a smooth, elliptical morphology with a pronounced central bulge. The light distribution is generally uniform with a gradual decrease in intensity from the core outwards, indicating a relatively old stellar population. The shape appears elongated, approximating a cigar-like form, suggesting it is an E5-E7 elliptical. No prominent spiral arms or dust lanes are visible. There may be some slight irregularities or minor disturbances in the outer regions, though these are subtle. The galaxy's color index suggests the stellar population is generally redder than that of spiral galaxies, though the central region appears slightly more yellow than the outer regions. There's no obvious evidence of recent major merger activity.
