This galaxy exhibits a moderately elongated morphology, appearing cigar-shaped and relatively smooth in texture. Its core exhibits a bright, concentrated luminosity, which gradually fades towards the outer edges. The color profile shows a warm hue, suggesting a population dominated by older stars. The smooth appearance and lack of obvious spiral arm structures suggest a classification toward the elliptical end of the Hubble sequence, although a faint disk may be present. There appears to be little evidence of significant recent merging activity or major disturbances to its structure, with most votes suggesting no merger. The mass estimates place this as a massive galaxy, but its star formation rate is low. Overall, the object appears to be a massive, relatively quiescent galaxy.
