The galaxy presents as a relatively smooth, elongated structure, possibly indicative of an elliptical morphology or a disk galaxy viewed at a significant angle. The central region exhibits a bright concentration of light, suggesting a dense stellar population or potentially an active galactic nucleus, although the resolution limits detailed analysis. The color profile appears to be predominantly redder in the main body of the galaxy, hinting at an older stellar population with a reduced rate of ongoing star formation. There is a bluer, more compact region located near the central core, possibly indicating a region of recent star formation. The overall structure shows some evidence of minor disturbance or irregularity, potentially suggesting past or ongoing interactions with another galaxy, although no clear merger features are readily apparent.
