The galaxy appears to be a relatively bright, well-defined elliptical galaxy with an overall smooth morphology. It exhibits a generally rounded shape, with a concentrated central bulge that is characterized by a yellowish hue, which may indicate an older stellar population dominating the galactic core. The galaxy's light profile seems to fade gradually from the core outwards, maintaining a consistent smooth texture across its observable extent. No significant indications of spiral arms, distinct dust lanes, or major disturbances are visible, which suggests the galaxy is not currently undergoing any major mergers or interactions. It is possibly an early-type galaxy with relatively low ongoing star formation, although a small amount of star formation in its past is possible.
