The galaxy presents as a somewhat amorphous, centrally concentrated structure with a subtle but noticeable disk-like component. It appears to exhibit a degree of structural disturbance, possibly indicative of a minor interaction or merger event in its recent history. There are hints of asymmetry in its shape and some irregularities in the overall light distribution. The galaxy's morphology is not perfectly smooth; it displays a level of textural detail that could arise from spiral arm segments, dust lanes, or tidal features. The color profile indicates a moderate population of older stars, possibly with pockets of ongoing or recent star formation that contribute to its observed hue. The galaxy's overall shape is closer to elliptical than a spiral type, with a suggestion of a faint tidal tail feature extending outward.
