The galaxy presents as a well-defined, moderately bright object with an elliptical morphology. Its core is highly concentrated and luminous, exhibiting a bright white-blue hue suggestive of a significant population of young, hot stars. Moving outwards from the central region, there's a gradual decrease in surface brightness into a less defined halo. The light distribution shows a smooth profile, indicating a relatively relaxed system, with a hint of a diffuse disk, possibly without prominent spiral arms. Overall, the galaxy appears as a relatively isolated system, with an estimated size of approximately 4 kiloparsecs based on a half-light radius. The color profile indicates that the galaxy is composed of older, redder stars in the outskirts. Evidence of interactions with nearby galaxies, such as tidal tails or distortions, are absent. There is an overall smooth structure.
