The galaxy presents as a somewhat elliptical structure with a concentrated central bulge exhibiting a yellowish hue. The disk appears relatively smooth, with a lack of prominent spiral arm structures or dust lanes discernable at this resolution. There appears to be a very slight flattening, suggesting it is closer to an E4 classification. The overall color profile leans towards redder wavelengths, with the outer regions appearing slightly bluer than the central bulge region. This could potentially indicate some ongoing star formation, especially given the slightly bluer colors present in the less dense regions. There are hints of minor disturbances or irregularities in the disk's structure, which may imply potential interaction events, although no clear merging features are obvious. The galaxy lacks significant morphological complexities.
