The galaxy presents as a centrally concentrated, luminous object with a smooth, elliptical morphology. The core exhibits a bright, diffuse glow, suggesting a high density of stars and possibly an active galactic nucleus, although the resolution is insufficient to confirm the presence of such a feature. The galaxy appears to be fairly evolved, given the lack of prominent spiral arms or distinct star-forming regions. The relatively uniform color profile, ranging from yellow to orange, is indicative of an older stellar population dominating the galaxy's light output. There are no obvious signs of recent major mergers, however the morphology is slightly disturbed, and there are some indications of minor tidal interactions or internal disturbances within the galaxy's outer regions. The galaxy is compact in size, and the smooth morphology indicates a relatively relaxed state in terms of star formation activity.
