The galaxy presents as a roughly elliptical structure with a distinct, concentrated central bulge. The bulge exhibits a reddish hue, indicative of an older stellar population and lower star formation activity in that region. Surrounding the bulge, a more diffuse disk is observed. This disk component displays a bluer color, suggesting the presence of younger, hotter stars and ongoing star formation. The galaxy appears to be relatively smooth, with no prominent spiral arms or bar structures immediately visible. There is some subtle indication of disturbances in the disk, perhaps minor tidal interactions. The galaxy's overall morphology points towards an intermediate classification, not a pure elliptical but also not a well-defined spiral galaxy.
