The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge and a gradually fading halo, suggesting an older stellar population. Color gradients appear minimal, with a slight reddening towards the core, indicative of a possible accumulation of older, redder stars in the central region. The overall shape is somewhat elongated, possibly deviating from a perfect sphere towards a cigar-like form, though no prominent spiral arm structures or dust lanes are discernible. There is a subtle asymmetry suggesting a past or ongoing minor interaction or disturbance. The galaxy appears relatively isolated with no major merging events currently in progress, though close inspection hints at possible tidal features or minor disturbances in the outer halo.
