This galaxy presents as a relatively smooth, elongated structure, appearing intermediate in shape between round and cigar-shaped. The central bulge exhibits a concentrated, luminous, and yellowish hue, potentially indicating an older stellar population. Moving outwards from the core, the galaxy displays a subtle disk-like feature, characterized by a bluish tint, suggesting the presence of younger stars and ongoing star formation. There's evidence of a minor disturbance, such as a slight asymmetry in the disk, indicative of past or ongoing gravitational interactions. Overall, the galaxy appears to be a relatively massive system with an active rate of star formation, exhibiting characteristics of both elliptical and spiral galaxies.
