The galaxy presents as a somewhat elongated, disk-like structure, viewed at an oblique angle, rather than face-on. The central region exhibits a concentrated, smooth appearance, displaying a bright, yellowish hue, suggestive of an older stellar population. Proceeding outward from this nucleus, the galaxy exhibits a transition to a bluer coloration, indicating the presence of younger stars or ongoing star formation, although at a low rate. Overall, the galaxy exhibits a relatively smooth texture, with no prominent spiral arms or distinct features immediately discernible. There is little evidence of any major disturbances or merging activity. The shape is closer to a cigar-shaped structure than perfectly round.
