The galaxy presents as a somewhat amorphous, though roughly elliptical, structure. Its core exhibits a concentrated luminosity, appearing yellowish-orange, which may indicate an older stellar population within the bulge. Extending outward from the central region, the galaxy shows diffuse, fainter features that could be indicative of a disk or spiral arms, although they are not clearly defined. These outer regions are slightly bluer in color, potentially suggesting regions of on-going star formation. The overall structure exhibits some signs of disturbance or interaction, as the morphology is not perfectly smooth and lacks clear symmetry. There appears to be a secondary, smaller object in close proximity, possibly interacting with the primary galaxy, which may contribute to the observed asymmetries and potential star formation.
