The galaxy appears to be a relatively smooth, elliptical system with a high degree of central concentration. The color profile is primarily yellow-orange, suggesting a dominant population of older stars and lower levels of ongoing star formation. The galaxy exhibits an elongated shape, approaching a cigar-like morphology. There is a suggestion of minor tidal disturbance or interaction, although the overall structure remains largely undisturbed. The galaxy does not appear to be undergoing a major merger, but exhibits some irregularity. Based on its size and apparent brightness, this galaxy is estimated to be relatively massive.
