The galaxy appears as an elliptical, cigar-shaped structure. A bright central bulge dominates the overall luminosity of the galaxy. Fainter, diffuse light extends outwards from the bulge, forming the main body of the galaxy. The color profile suggests a relatively homogenous stellar population, with a slight reddening apparent at the galaxy's periphery. The shape deviates moderately from a perfect ellipse, with a ratio of the major axis to the minor axis of approximately 4:1, possibly indicating a mild degree of disturbance or tidal interaction, although no obvious companion galaxies or tidal tails are visible within the immediate field of view. Star formation is subdued with a small fraction of disk light, and any spiral arm structures are not detectable. 
