The galaxy presents a largely smooth morphology with hints of a disk-like structure. The central region exhibits a bright, concentrated luminosity, likely indicating a substantial galactic nucleus. The color profile suggests a relatively old stellar population, with a tendency towards redder hues. The galaxy's overall shape appears to be somewhere between round and elongated, not quite cigar-shaped. There's no clear evidence of major disturbances or merging events, although subtle irregularities in the outer regions could imply minor tidal interactions or past accretion events. Based on the light profile, ongoing star formation is likely modest.
