The galaxy presents an elliptical morphology, exhibiting a moderately elongated shape. Its light profile appears relatively smooth, lacking prominent spiral arms or a distinct bar structure. The color distribution indicates a population dominated by older stars, with a yellowish-red hue, although there is a bluer, star-forming region on the edge of the galaxy. This implies that star formation is still ongoing within the galaxy, though perhaps at a lower rate than in actively star-forming spiral galaxies. The galaxy appears isolated, with no obvious signs of interaction or recent merger events, though there is a small irregular galaxy nearby. Overall, this galaxy appears to be a moderately massive system, possibly in a transitional stage between a blue, star-forming galaxy and a red, quiescent galaxy.
