The galaxy presents a morphology consistent with a late-type spiral galaxy. The central bulge appears quite bright and concentrated, indicating a significant stellar population density. The disk appears less prominent, with a relatively smooth texture and subtle hints of spiral arm structure extending outwards. The overall color of the galaxy appears to be tending towards the redder end of the spectrum, particularly within the bulge. The galaxy appears to be relatively isolated, with no major signs of ongoing mergers or significant tidal disturbances. The shape tends towards an elliptical-like shape. The galaxy is of moderate size, with a concentrated central light profile which suggests a somewhat older stellar population within its nucleus. Star formation rates appear to be relatively low given the red hue.
