The galaxy appears as a relatively smooth, elliptical shape, with a concentrated central bulge. Its color is generally redder, indicative of an older stellar population and lower star formation rate. The galaxy exhibits an elongated morphology, leaning towards a cigar shape. The light distribution appears to be somewhat disturbed, possibly showing signs of a minor interaction or internal instabilities. There is no clear evidence of spiral arms or a prominent disk structure. The galaxy does not appear to be undergoing a major merger event.
