The galaxy presents as a relatively smooth, elliptical structure. Its overall shape appears moderately elongated, approaching a cigar-like morphology, though it primarily resides closer to an in-between classification between perfectly round and elongated. The central region exhibits a bright, concentrated luminosity, suggesting a prominent galactic nucleus. The color profile appears to be dominated by warmer tones, trending towards the redder end of the spectrum. This coloration may be indicative of an older stellar population. No distinct spiral arms or significant dust lanes are readily apparent, supporting the smooth classification. There is no apparent evidence of a major merger event or significant disturbances in its structure. Possible minor disturbances cannot be ruled out, but are not obvious.
