This galaxy presents as a somewhat asymmetrical system. There is a central, roughly spherical, bright bulge component, with a yellowish hue. This may suggest an older stellar population within the bulge. Extending from this central region, there is a noticeable, elongated feature or arm. This appendage exhibits a reddish color gradient that becomes more prominent towards the extension's distal end, possibly indicating the presence of dust lanes, or recent star formation. The overall shape suggests a disk component, although not a well-defined spiral structure is visible. The system may be experiencing some form of tidal interaction or disturbance, given the asymmetry and arm structure. The lack of a clear, organized spiral pattern suggests that the system may be undergoing a merger event, or has experienced one in the past. Further spectroscopic analysis is needed to confirm this.
