The galaxy presents an overall smooth morphology, suggestive of an elliptical type or possibly a lenticular galaxy seen at an oblique angle. The core exhibits a concentrated, yellowish-orange hue, indicative of an older stellar population. Surrounding the core, a slightly bluer halo is observed, gradually fading into the background. No distinct spiral arms or prominent dust lanes are discernible. The shape is somewhat elongated but is closer to being round than cigar shaped. There appear to be minor disturbances. This galaxy is actively forming stars at a modest rate. The galaxy appears to be of intermediate mass.
