The galaxy presents as a somewhat elongated, faint object, exhibiting a blueish-white hue across its structure. The morphology is suggestive of a disk-like system viewed at an oblique angle, although no distinct spiral arm structure is discernible. The color profile suggests ongoing or recent star formation, particularly concentrated within the central regions and extending along the apparent major axis. The overall smooth appearance indicates a relatively evolved system, potentially with a dominant bulge or spheroid component in addition to the disk. There is a slight distortion or irregularity in the galaxy's shape, possibly indicative of tidal interactions with a smaller companion, or perhaps due to a recent merger event. Overall, this appears to be a low-mass galaxy.
