The galaxy presents as a relatively smooth, elliptical-like structure. There is a slight elongation, with an approximate cigar shape. The light is concentrated in the center, suggesting a prominent bulge. The galaxy exhibits a reddish hue overall, indicative of an older stellar population and lower rates of star formation. There appears to be no distinct spiral arm structure or significant dust lanes visible. The galaxy does not appear to be undergoing any major merging activity, although there is potentially some minor disturbance in the outer regions. The smooth appearance suggests a classification towards an elliptical or lenticular galaxy type.
