The galaxy presents as a moderately inclined disk system. A bright, concentrated central bulge dominates the core region, exhibiting a yellowish-white hue, suggestive of an older stellar population. The surrounding disk appears bluer in color, indicating the presence of younger, hotter stars and potentially ongoing star formation. The disk structure appears relatively smooth with no clear evidence of spiral arm structure. The galaxy does not show strong signs of tidal disturbances or interactions, indicating it is a relatively isolated system currently undergoing quiescent evolution. The shape is ellipsoidal, with a ratio of major to minor axis of approximately 2:1. Overall, the galaxy presents characteristics of a late-type disk galaxy with a significant bulge component, transitioning towards a more quiescent state.
