The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The color profile exhibits a yellowish-red hue concentrated in the core, gradually fading to a bluer tint in the outer regions. The overall shape appears to be somewhat elongated, but not markedly cigar-shaped, suggesting a moderate ellipticity. There is no obvious evidence of major disturbances or ongoing mergers from visual inspection, though subtle features might be present upon further analysis. The galaxy's size appears modest. Based on the observed colors, the galaxy likely contains a mix of stellar populations with potentially older, redder stars dominating the core. The bluer outskirts may indicate some ongoing, though likely subdued, star formation.
