The galaxy appears as a somewhat elliptical, moderately bright object with a relatively smooth texture. The central region presents a concentrated luminosity, suggesting a significant stellar density, possibly an aging population of stars. Moving outward from the center, the light diminishes gradually with no defined spiral arm structure visible in this image.

The galaxy's color profile reveals a generally yellow-white hue concentrated in the center, which could indicate the presence of older stars. Fainter blue tinges are observed across the galaxy. These areas may indicate regions of more recent, but limited, star formation. There are no obvious signs of substantial dust lanes or regions of intense, ongoing star formation, nor is there evidence of a significant tidal disturbance. The overall impression is that of a reasonably evolved system experiencing, at most, minor activity.
