The galaxy presents as a relatively smooth, elliptical structure. The light distribution suggests a concentrated central bulge that diminishes gradually towards the edges. The galaxy's overall shape is elongated, approximating a cigar-like form. There are no obvious signs of spiral arm structure or intense star-forming regions. The color profile indicates a dominant population of older stars. No prominent tidal features or major distortions suggestive of recent mergers are apparent, although there is some minor asymmetry in the outer regions. The galaxy appears relatively isolated and undisturbed.
