The galaxy presents a predominantly smooth morphology, with a high degree of central concentration. Its overall shape approximates a spheroid, exhibiting significant circularity with minimal deviation towards a cigar-like form. The light distribution suggests a relatively old stellar population dominating the galaxy's composition, based on its color. There is a notable absence of prominent spiral arms or significant dust lanes. No obvious signs of a major ongoing merger event are present, although minor disturbances cannot be ruled out based on visual inspection alone. The color profile indicates a generally redder, more evolved stellar population. Star formation activity appears to be suppressed.
