The galaxy presents as a generally smooth, elongated structure, suggesting a classification leaning toward elliptical. It exhibits a concentrated central bulge with a gradual decline in luminosity towards its outer edges. The primary color is a warm, yellowish-orange hue, indicative of an older stellar population and diminished ongoing star formation. The galaxy's shape appears somewhat cigar-shaped, lacking a well-defined spiral arm structure. There is no apparent dust lane visible. Subtle asymmetry is present, potentially resulting from a minor gravitational interaction, though no major disruption is immediately evident. The overall appearance suggests a galaxy of substantial mass with relatively quiescent star-forming activity.
