The galaxy exhibits a pronounced elongated, cigar-shaped morphology. It presents a relatively smooth appearance, with a concentrated central bulge region exhibiting a yellowish-orange hue, suggesting an older stellar population. Fainter, somewhat diffuse, bluer features extend from the central region towards the galaxy's edges, potentially indicating regions of more recent star formation within a disk-like component. There are indications of possible disturbances in the overall structure, such as faint asymmetries that could be indicative of a past or ongoing interaction or merger event. Overall, this appears to be a substantial galaxy at a considerable distance, exhibiting a combination of evolved and actively star-forming regions and some possible interaction.
