The galaxy presents as a concentrated aggregation of light, exhibiting a generally elliptical morphology. Its central region appears smooth and featureless, suggesting a relatively old stellar population. The galaxy's light profile appears diffuse, indicating a well-mixed distribution of stars within the galactic body. There is little evidence of spiral arm structure or prominent dust lanes; the overall appearance aligns with an early-type galaxy classification. The apparent color is slightly redder than average, which would be expected for an older population of stars. The galaxy does not appear to be undergoing any major merging events. Small irregularities are observed, possibly indicative of minor interactions or internal disturbances. The physical scale is approximately 5 kpc, so it's a relatively small galaxy. The stellar mass is quite large for the size. Star formation is slow. The morphology is primarily smooth, with a round to intermediate shape.
